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Whole Heliosphere Interval: Overview of JD16

Published online by Cambridge University Press:  21 October 2010

David F. Webb ,
Sarah E. Gibson  and
Barbara J. Thompson
David F. Webb
Affiliation:
ISR, Boston College, Institute for Scientific Research, 140 Commonwealth Ave., Chestnut Hill, MA 02467 Also at: Air Force Research Laboratory, Hanscom AFB, MA, 01731-3010, USA email: david.webb@hanscom.af.mil
Sarah E. Gibson
Affiliation:
HAO/NCAR, P.O. Box 3000, Boulder, CO 80301-3000, USA email: sgibson@ucar.edu
Barbara J. Thompson
Affiliation:
NASA/Goddard Space Flight Center, Greenbelt, MD 20771, USA email: barbara.j.thompson@nasa.gov
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Abstract

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The Whole Heliosphere Interval is an international observing and modeling effort to characterize the three-dimensional interconnected solar-heliospheric-planetary system, i.e., the “heliophysical” system. WHI was part of the International Heliophysical Year, on the 50th anniversary of the International Geophysical Year, and benefited from hundreds of observatories and instruments participating in IHY activities. WHI describes the 3-D heliosphere originating from solar Carrington Rotation 2068, March 20–April 16, 2008. The focus of IAU JD16 was on analyses of observations obtained during WHI, and simulations and modeling involving those data and that period. Consideration of the WHI interval in the context of surrounding solar rotations and/or compared to last solar minimum was also encouraged. Our goal was to identify connections and commonalities between the various regions of the heliosphere.

Keywords

Sun: magnetic fieldsSun: coronal mass ejections (CMEs)interplanetary (IP) medium(Sun:) solar-terrestrial relations
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Highlights H15: Highlights of Astronomy , November 2009 , pp. 471 - 479
Copyright
Copyright © International Astronomical Union 2010

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